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一种新型暗物质与银河系和仙女座星系大旋转曲线的比较。

Comparison of a new type of Dark Matter with the Milky Way and M31 grand rotation curves.

作者信息

Law Bruce M

机构信息

Department of Physics, Kansas State University, 116 Cardwell Hall, Manhattan, KS, 66506-2601, USA.

出版信息

Sci Rep. 2024 Oct 15;14(1):24090. doi: 10.1038/s41598-024-74884-6.

DOI:10.1038/s41598-024-74884-6
PMID:39406824
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC11480391/
Abstract

In the electron Born self-energy (eBse) model, free electrons are of finite-size and possess both a rest mass, m, as well as, a Born mass, m = 74,000 m. The Born mass, which originates from the energy contained within the electric field that surrounds a finite-sized electron, serves as a Dark Matter (DM) particle in this theory (designated eBDM, electron Born Dark Matter). The equation of state for m is w = -1, which implies that two Born masses experience a repulsive gravitational interaction. This repulsive gravitational interaction stabilizes the formation of a DM halo of m particles, of typical halo size ~ 100 kpc, around a central mass M (e.g. a galaxy), where this gravitational stability arises from the competing attractive M - m and repulsive m - m interactions. A solution of the linearized Poisson-Boltzmann equation, for this system, allows one to derive an expression for the rotational velocity V(R), as a function of radius R from the galactic center. A composite model composed of rotational velocity contributions from the galactic bulge, galactic disk, as well as, V(R) is found to provide a good description of the Grand Rotation Curves for the Milky Way and M31 galaxies.

摘要

在电子玻恩自能(eBse)模型中,自由电子具有有限大小,且既有静止质量(m),又有玻恩质量(m = 74000m)。玻恩质量源自围绕有限大小电子的电场所含能量,在该理论中作为暗物质(DM)粒子(称为eBDM,即电子玻恩暗物质)。(m)的状态方程为(w = -1),这意味着两个玻恩质量会经历排斥性引力相互作用。这种排斥性引力相互作用稳定了(m)粒子组成的暗物质晕的形成,典型晕大小约为(100)千秒差距,围绕中心质量(M)(如星系),其中这种引力稳定性源于吸引性的(M - m)相互作用与排斥性的(m - m)相互作用之间的竞争。对于该系统,线性化泊松 - 玻尔兹曼方程的一个解使人们能够推导出作为到星系中心距离(R)的函数的旋转速度(V(R))的表达式。由星系核球、星系盘以及(V(R))的旋转速度贡献组成的复合模型,被发现能很好地描述银河系和M31星系的总旋转曲线。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/3752/11480391/513d88ff278e/41598_2024_74884_Fig6_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/3752/11480391/8ade51fce096/41598_2024_74884_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/3752/11480391/e5650cc3d13e/41598_2024_74884_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/3752/11480391/8da4c2d46b17/41598_2024_74884_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/3752/11480391/1d914d8981e5/41598_2024_74884_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/3752/11480391/7da335b559e5/41598_2024_74884_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/3752/11480391/513d88ff278e/41598_2024_74884_Fig6_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/3752/11480391/8ade51fce096/41598_2024_74884_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/3752/11480391/e5650cc3d13e/41598_2024_74884_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/3752/11480391/8da4c2d46b17/41598_2024_74884_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/3752/11480391/1d914d8981e5/41598_2024_74884_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/3752/11480391/7da335b559e5/41598_2024_74884_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/3752/11480391/513d88ff278e/41598_2024_74884_Fig6_HTML.jpg

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